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Assessment of the performance of GPS/Galileo PPPRTK convergence using ionospheric corrections from networks with different scales
Earth, Planets and Space volume 74, Article number: 47 (2022)
Abstract
The rapid convergence of precise point positioning realtime kinematics (PPPRTK) with centimeterlevel accuracy is of utmost importance for many applications. One way of accelerating this convergence is to explore the use of ionospheric models and multiple global navigation satellite system (GNSS) observations, e.g., Global Positioning System (GPS) and Galileo Satellite Navigation System (Galileo) observations. Because the temporal and spatial variations of the ionosphere are significant, convergence analysis of PPPRTK should be investigated in networks with different scales, especially networks with large differences in their scales. This study describes the convergence performance of PPPRTK using GPS/Galileo observations derived from networks with different scales under medium ionospheric conditions. Slant ionospheric corrections were first estimated from the reference network and then imported as virtual observations to enhance the convergence performance of PPPRTK at the user interface. The results show that for the 165km reference site spacing, the portions of singledifferenced (SD) ionospheric residuals within 0.3 total electron content units (TECU) were 85.2% and 81.7% for the GPS and Galileo observations, respectively. Considering the 90th percentile of horizontal position errors, the PPPRTK convergence time within the network with 165km spacing was shortened from 2.5 min for GPSonly observations to 2.0 min for integrated GPS + Galileo observations. For the network of about 50 km, the proportions of the SD ionospheric residuals of the GPS and Galileo constellation within 0.3 TECU were 95.9% and 82.8%, respectively. The PPPRTK convergence time of the 90th percentile horizontal positioning errors based on GPSonly observations was 2.0 min but 1.5 min based on integrated GPS + Galileo observations. Using GPS and Galileo observations, the convergence time could be reduced by 25% for the network with 50km spacing. Our results suggest that the convergence time of PPPRTK depends on the scale of the reference network and becomes shorter as the scale of the network decreases. Compared with the GPSonly PPPRTK, the GPS/Galileo PPPRTK could shorten the convergence time further.
Graphical Abstract
Introduction
In the past few years, precise point positioning (PPP) has become a widely applied method for providing precise positioning due to its convenience and efficiency (Zumberge et al. 1997; Kouba and Heroux 2011). Unfortunately, the convergence time of conventional PPP is still half an hour or longer. To reduce the convergence time and improve positioning accuracy, several PPP ambiguity resolution (AR) approaches have been proposed in the past few years to restore the integer feature of ambiguities (Ge et al. 2008; Collins 2008; Laurichesse et al. 2009; Mervart et al. 2008; Bertiger et al. 2010; Teunissen et al. 2010; Geng et al. 2012; Loyer et al. 2012). The relationship between these methods has also been demonstrated (Geng et al. 2010a; Shi and Gao 2014; Teunissen and Khodabandeh 2015). However, fast and reliable ambiguity resolution is still not available due to the obstacle of atmospheric errors, especially ionospheric delays. In such cases, a novel technology called PPP realtime kinematic (PPPRTK) has been proposed (Wubbena et al. 2005; Teunissen et al. 2010; Mervart et al. 2008; Geng et al. 2011). PPPRTK utilizes the precise atmospheric corrections generated from the reference network to accelerate the ambiguity resolution. Moreover, the PPPRTK technique also has the advantage of low bandwidth requirements and oneway communication, thus providing a promising opportunity for the emerging mass market and automotive applications.
Benefiting from the unique advantages of PPPRTK, great efforts in recent years have been focused on PPPRTK with promising results, both in research as well as in applications (Li et al. 2011, 2020; Zhang et al. 2011; Odijk and Zhang 2012; Psychas and Verhagen 2020; Nadarajah et al. 2018; Ma et al. 2020). Li et al. (2011) implemented a regional augmentation PPP experiment in a network with an average distance of about 60 km. The results showed that an almost instantaneous ambiguity resolution of global positioning system (GPS) PPP was available if the interpolated atmospheric corrections derived from the reference stations could be obtained. Zhang et al. (2011) tested two GPS CORS networks with an average distance ranging from 60 to 100 km. The results demonstrated the performance of ambiguity fixing and positioning accuracy have achieved ideal effects. Odijk and Zhang (2012) performed the singlefrequency PPPRTK using a geodetic receiver as well as a lowcost receiver. The results showed that the cmlevel positioning accuracy can be obtained by utilizing the atmospheric corrections of the reference networks and observations of less than 10 min. Psychas and Verhagen (2020) demonstrated that subdecimeter horizontal positioning accuracy could be achieved almost instantaneously for a network with 68km spacing. However, when the interstation distance is increased to 237 km, it required about 7.0 min to achieve a subdecimeter horizontal positioning accuracy when only GPS observations were used. Currently, the rapid development of multiconstellation global navigation satellite systems (GNSS) has created new opportunities for PPPRTK. Li et al. (2020) investigated the performance of GPS/BeiDou Navigation Satellite System (GPS/BDS) PPPRTK. The results revealed that PPPRTK fixed solutions could be achieved in an average of 1.5, 1.6, and 1.2 epochs, and the corresponding positioning rootmeansquare (RMS) in the east, north, and vertical components was 0.80, 0.47, and 1.97 cm for GPS alone; 0.98, 0.73, and 2.97 cm for BDS alone; and 0.56, 0.35, and 2.33 cm for integrated GPS + BDS observations. Nadarajah et al. (2018) used the GPS, BDS, and Galileo Satellite Navigation System (Galileo) observations to investigate the positioning and convergence performance of PPPRTK scenarios. The results indicated that with a regional network of about 30 km, subdecimeter positioning accuracy in the horizontal and vertical components could be achieved within 4.5 and 5.0 min for GPS alone and 1.0 and 0.5 min for integrated multiGNSS (GPS, BDS, and Galileo) observations. Ma et al. (2020) investigated multiGNSS PPPRTK in the local area. Their results showed that the multiGNSS observations could accelerate the ambiguity resolution of PPP for GPS alone. Unfortunately, they investigated the positioning and convergence performance without utilizing ionospheric corrections.
Despite much work having been devoted to investigating the impact of ionospheric corrections for PPPRTK performance (e.g., multiGNSS PPPRTK and multiscale PPPRTK), there are still some potential problems that need to be further researched and clarified. For instance, Psychas and Verhagen (2020) investigated regional augmented PPP AR by utilizing ionospheric corrections derived from networks with different scales. However, only GPS observations were used to generate the ionospheric delays and to investigate the positioning and convergence performance of PPPRTK. Thus, they did not explore the impact of multiGNSS observations on PPPRTK performance and the accuracy of ionospheric delays in networks with different scales. Although multiscale PPPRTK using multiGNSS observations was also investigated, Nadarajah et al. (2018) only demonstrated regional augmented PPP AR in smallscale reference networks and did not explore the regional augmented PPP AR for networks with large differences in scale.
As indicated by previous studies, the ionospheric delays derived from the regional GNSS network play an important role in PPPRTK for accelerating ambiguity resolution. However, the spatial resolution and accuracy of the generated ionospheric corrections are associated with the scale of the reference network and the stations’ distribution in a network. This may affect its performance in PPPRTK when adopted as an accurate prior constraint. Furthermore, current research concerning multiGNSS PPPRTK has mostly used smallscale networks, with the aim of investigating the convergence and positioning performance. The performance of multiGNSS PPPRTK with ionospheric corrections derived from networks with large differences in their scales still needs further investigation. For this reason, this study aimed to systematically analyze the convergence performance of PPPRTK using the ionospheric corrections of GPS and the Galileo constellation derived from networks with large differences in their scales.
The remainder of this study is organized as follows. “Methods” section introduces the uncombined PPP (UCPPP) AR algorithm and then describes the estimation, representation, and constraint methods of ionospheric correction. The design of the PPPRTK platform software system is also presented in this part as well. “Results” section outlined the strategies used for data processing and focuses on the assessment of the convergence performance of PPPRTK utilizing GPS/Galileo observations from two networks with different scales. In “Discussion” section, some conclusions and perspectives are provided.
Methods
In this section, the mathematical models for undifferenced and uncombined PPPRTK are summarized first, followed by an investigation of the methods that can generate and interpolate slant ionospheric delays; next, the augmented PPP model is discussed. The comprehensive data processing strategies are also presented as well.
UCPPP observation equations
The original observation equations for the dualfrequency pseudorange and carrier phase observations are given as:
where \(P_{1}\) and \(P_{2}\) denote the pseudorange measurements and \(L_{1}\) and \(L_{2}\) are carrier phase measurements on the two frequencies which are actually L_{1}, L_{2} for GPS, and E1, E5a for Galileo; \(\rho\) is the distance between the antenna phase center of both the satellite and receiver corrected for many errors, including phase windup, Shapiro signal propagation delay, solid and ocean tides, pole tides, relativistic effect, antenna phase center offsets (PCOs), and phase center variations (PCVs) for the satellite and receiver; \({\text{dt}}^{{\text{r}}}\) and \({\text{dt}}^{{\text{s}}}\) are the clock offsets of the satellite and receiver, respectively; \(c\) is the speed of light in a vacuum; \(T\) is the total troposphere delay (m); \(I_{1}\) represents the slant ionospheric delay at frequency L_{1} (m); \(N_{1}\) and \(N_{2}\) are the ambiguity parameters at frequency (k = 1, 2); \(\lambda_{k}\) denotes the wavelength at frequency k (k = 1, 2); \(\varepsilon_{{P_{k} }}\) and \(\varepsilon_{{L_{k} }}\) are the measurement noise and multipath effect for the pseudorange and carrier phase measurements at frequency k (k = 1, 2), respectively; \(D_{{P_{k} }}^{{\text{r}}}\) and \(D_{{P_{k} }}^{{\text{s}}}\) are the pseudorange hardware delay of the receiver and satellite at frequency k (k = 1, 2), respectively; \(B_{{L_{k} }}^{{\text{r}}}\) and \(B_{{L_{k} }}^{{\text{s}}}\) are the carrier phase hardware delay of the receiver and satellite at frequency k (k = 1, 2), respectively; and \(\gamma_{2} = \frac{{f_{1}^{2} }}{{f_{2}^{2} }}\), where \(f_{k}\) denotes the frequency k (k = 1, 2).
If we consider the ionospheric free (IF) satellite clocks, the UCPPP model can be reparametrized as (Laurichesse and Privat 2015; Xiang et al. 2020):
where \(D_{{P_{{{\text{IF}}}} }}^{{\text{r}}}\) and \(D_{{P_{{{\text{IF}}}} }}^{{\text{s}}}\) represent the pseudorange hardware delay based on the ionospheric free combination for the receiver and satellite, respectively; \({\text{DCB}}_{{P_{1}  P_{2} }}^{{\text{r}}}\) and \({\text{DCB}}_{{P_{1}  P_{2} }}^{{\text{s}}}\) represent the P_{1}/P_{2} signals differential code biases (DCBs) of the receiver and satellite, respectively; \(\tilde{N}_{1} = N_{1} + B_{{L_{1} }}^{{\text{r}}}  B_{{L_{1} }}^{{\text{s}}}  {{\left( {c(D_{{P_{{{\text{IF}}}} }}^{{\text{r}}}  D_{{P_{{{\text{IF}}}} }}^{{\text{s}}} ) + \frac{{f_{2}^{2} }}{{f_{1}^{2}  f_{2}^{2} }}\left( {{\text{DCB}}_{{P_{1}  P_{2} }}^{{\text{r}}}  {\text{DCB}}_{{P_{1}  P_{2} }}^{{\text{s}}} } \right)} \right)} \mathord{\left/ {\vphantom {{\left( {c(D_{{P_{{{\text{IF}}}} }}^{{\text{r}}}  D_{{P_{{{\text{IF}}}} }}^{{\text{s}}} ) + \frac{{f_{2}^{2} }}{{f_{1}^{2}  f_{2}^{2} }}\left( {{\text{DCB}}_{{P_{1}  P_{2} }}^{{\text{r}}}  {\text{DCB}}_{{P_{1}  P_{2} }}^{{\text{s}}} } \right)} \right)} {\lambda_{1} }}} \right. \kern\nulldelimiterspace} {\lambda_{1} }}\) is the floating narrowlane (NL) ambiguity (cycles) containing the biases of both the carrier phase and the pseudorange; \(\tilde{N}_{2} = N_{2} + B_{{L_{2} }}^{{\text{r}}}  B_{{L_{2} }}^{{\text{s}}}  {{\left( {c(D_{{P_{{{\text{IF}}}} }}^{{\text{r}}}  D_{{P_{{{\text{IF}}}} }}^{{\text{s}}} ) + \frac{{f_{1}^{2} }}{{f_{1}^{2}  f_{2}^{2} }}\left( {{\text{DCB}}_{{P_{1}  P_{2} }}^{{\text{r}}}  {\text{DCB}}_{{P_{1}  P_{2} }}^{{\text{s}}} } \right)} \right)} \mathord{\left/ {\vphantom {{\left( {c(D_{{P_{{{\text{IF}}}} }}^{{\text{r}}}  D_{{P_{{{\text{IF}}}} }}^{{\text{s}}} ) + \frac{{f_{1}^{2} }}{{f_{1}^{2}  f_{2}^{2} }}\left( {{\text{DCB}}_{{P_{1}  P_{2} }}^{{\text{r}}}  {\text{DCB}}_{{P_{1}  P_{2} }}^{{\text{s}}} } \right)} \right)} {\lambda_{2} }}} \right. \kern\nulldelimiterspace} {\lambda_{2} }}\) is the floating ambiguity at a frequency of 2 (cycles) containing the biases of both the carrier phase and the pseudorange; and \(\tilde{N}_{{\text{W}}} = \tilde{N}_{2}  \tilde{N}_{1}\) is the floating widelane (WL) ambiguity (cycles) containing the biases of both the carrier phase and the pseudorange.
If known satellite clock corrections and DCBs are used to correct the observation equations of the UCPPP model, the corresponding simplified formulae read:
where \(\widetilde{{{\text{dt}}}}^{{\text{r}}} = {\text{dt}}^{{\text{r}}} + D_{{P_{{{\text{IF}}}} }}^{{\text{r}}} ;\) \(\tilde{I}_{1} = I_{1}  \frac{{f_{2}^{2} }}{{f_{1}^{2}  f_{2}^{2} }}{\text{DCB}}_{{P_{1}  P_{2} }}^{{\text{r}}} .\)
If the UCPPP model can be corrected by utilizing the satellite DCBs, and if external ionospheric products are not available, the ionospheric delays contaminated by the receiver’s DCBs will be considered as an unknown parameter to be estimated. This way, the state vector of unknowns is \(\vec{X} = \left[ {\begin{array}{*{20}c} x & y & z & {\widetilde{{{\text{dt}}}}^{{\text{r}}} } & T & {\tilde{I}_{1} } & {\tilde{N}_{1} } & {\tilde{N}_{{\text{W}}} } \\ \end{array} } \right]^{{\text{T}}}\), which will be estimated by the UCPPP model using a Kalman filter approach. The slant ionospheric corrections can be generated only when the WL and NL ambiguity can be fixed successfully.
The observation equations of the UCPPP model above can be applied to the entire PPPRTK network and the user components. Additionally, for the network component, the station coordinates should be fixed to the true values to accelerate the convergence for the estimated parameters in the PPP filter. However, the user’s receiver positions have to be estimated to evaluate the convergence performance in the user components.
UCPPP AR
Since satellites’ pseudorange and carrier phase bias products have been made available by GNSS analysis centers, satellites’ pseudorange biases can be corrected by DCBs or observable specific signal biases (OSBs), and carrier phase biases can be corrected by uncalibrated phase delays (UPDs) or OSBs (Banville et al. 2020; Liu et al. 2021). According to Eq. (3), the pseudorange and carrier phase biases from receivers are mainly absorbed by ambiguities, slant ionospheric delays, and receiver clock offsets. Thus, the satellitedependent biases could be removed in advance; instead, singledifference (SD) ambiguities between satellites had to be formed to remove the biases of the receiver components. Specifically, we have chosen the satellite with the highest elevation as the reference satellite and found the single difference between the reference satellite and other satellites in the same satellite system (Li et al. 2016).
The PPP AR algorithm is divided into two key steps. Firstly, the SD WL ambiguities can be resolved by rounding. The equation for calculating the probability \(P_{0}\) of fixing SD WL ambiguity is given as (Dong and Bock 1989):
where \(P_{{0}}\) represents the probability of fixing SD WL ambiguity; \(B\) and \(\delta\) represents the floating SD WL ambiguity and its accuracy, respectively; and \(n\) denotes the nearest integer of \(B.\)
The fixed SD WL ambiguities are then considered as virtual observations to update the remaining unknowns and variance–covariance matrix to enhance the fixing of SD NL ambiguities. The optimal integer solution for SD NL ambiguities can be found by applying the leastsquare ambiguity decorrelation adjustment (LAMBDA) method (Teunissen 1995). Since the residual model errors can affect the fractional part of SD NL ambiguities, ambiguity validation is particularly important to fix SD NL ambiguities reliably (Ge et al. 2008; Cui et al. 2021). Specifically, for ambiguity validation, the ratio and bootstrapping success rate are frequently utilized for AR (Ji et al. 2010; Verhagen 2005, 2003; Li and Zhang 2015). The bootstrapping success rate can be applied here. It has been regarded as a lower bound for the integer leastsquares (ILS) success rate (Teunissen 1998; Blewitt 1989). However, the computed success rate always cannot objectively reflect the real success rate of actual observations although the computed success rate could still be high (Li and Zhang 2015). Meanwhile, the threshold of ratio is only determined by the simulated measurements at present, so the empirical value cannot be efficiently applied to validate the ambiguity resolution (Blewitt 1989). Furthermore, when the data are initialized or the satellite elevation is too low, it is difficult to accurately fix ambiguities due to the low accuracy. Therefore, it is essential to apply strict quality control strategies for the determination of the ambiguity subset, which is a special case of integeraperture estimation (Teunissen 2005).
The detailed quality control parameters of UCPPP AR used in this study are listed in Table 1.
Figure 1 shows the flowchart of the UCPPP AR algorithm. First, the subset of SD WL ambiguities was determined carefully. Next, the SD WL ambiguities were first fixed by the rounding method in a onestep approach and applied as a constraint to update the normal equations of the UCPPP model. Afterwards, the LAMBDA algorithm was applied to fix the subset of SD NL ambiguities in a twostep approach. In particular, we require at least four resolved ambiguities for partial ambiguity fixing. If the number of ambiguities was less than four or if partial ambiguity fixing could pass the threshold of either the onestep or twostep approach, we kept the floating solutions instead and moved on to the next epoch.
Estimation, representation, and constraint of ionospheric corrections
To provide precise ionospheric corrections for users, proper derivation and representation of ionospheric corrections play a critical role in the positioning performance of PPPRTK. In our study, the precise slant ionospheric delays were derived from the UCPPP model with a fixed ambiguity method. In fact, because of the impact of UPDs, the undifference (UD) ambiguity and SD ambiguity are no longer integers (Blewitt 1989). The removal of UPDs from both satellite and receiver is essential for PPPAR to recover the ambiguity’s integer property. Proceeding this way, when satellitedependent UPDs can be corrected by applying OSBs/UPDs products, and receiverdependent UPDs can be eliminated by SD ambiguities between satellites, the integer property of the SD ambiguities between satellites will be retrieved.
At the reference sites, the SD WL ambiguities are fixed first. After the SD WL ambiguities have been fixed successfully, the fixed SD WL ambiguities are considered as constraints to update the floating solutions. Afterwards, the UD NL ambiguities are extracted from the floating solutions updated with the fixed SD WL ambiguities. The UD NL ambiguities can be transformed to SD NL ambiguities. After the SD NL ambiguities have been fixed successfully, the state vector of the floating solutions is updated with the fixed SD NL ambiguities again.
The state vector of the floating solutions can be updated with the following formula (Li et al. 2014a).
where \(\mathop {N_{{{\text{SD}}}} }\limits^{ \wedge }\) represents the SD floating ambiguity that can be accurately fixed; \(\mathop {N_{{{\text{SD}}}} }\limits^{ \vee }\) is the optimal integer solution for SD floating ambiguity; \(Q_{{\mathop N\limits^{ \wedge } \mathop N\limits^{ \wedge } }}\) denotes the UD floating ambiguity covariance matrix that determines the structure of \(\mathop {N_{{{\text{SD}}}} }\limits^{ \wedge } ;\) \(Q_{{\mathop X\limits^{ \wedge } \mathop N\limits^{ \wedge } }}\) represents the covariance matrix involving the relationship between the UD floating ambiguity and the remaining estimated parameters of the floating solutions; \(S\) represents the transformation matrix that maps from the UD floating ambiguity to the SD floating ambiguity; \(\mathop X\limits^{ \wedge }\) and \(\mathop X\limits^{ \vee }\) denote the vector of both the floating and the fixed solution containing the remaining unknowns, respectively; \(Q_{{\mathop X\limits^{ \wedge } \mathop X\limits^{ \wedge } }}\) and \(Q_{{\mathop X\limits^{ \vee } \mathop X\limits^{ \vee } }}\) are the covariance matrix of both the floating and the fixed solution containing the remaining unknowns, respectively.
After the ionospheric corrections have been generated from the reference network, the interpolation method is recommended for many algorithms (Han 1997; Wanninger 1995; Gao et al. 1997). Because the variance of interpolated errors mainly depends on the distance between stations, we interpolated the slant ionospheric delay by applying the distancebased linear interpolation method (DIM) for the same satellite to enhance the convergence performance of PPPRTK. Throughout the DIM algorithm, slant ionospheric correction of a satellite s visible by the user component is interpolated from \(n\) reference stations and weighted by the inverse distance between the reference network and the user components. The interpolated slant ionospheric correction can be calculated as follows:
where \(d_{i}\) denotes the distance between the reference station and user station, \(I_{{\text{u}}}^{{\text{s}}}\) represents the interpolated slant ionospheric correction of satellite s visible to the user, \(I_{i}^{{\text{s}}}\) is the pure slant ionospheric delay of satellite s visible to the user and reference station i, \(\tilde{I}_{i}^{{\text{s}}}\) is the slant ionospheric delay containing the \(I_{i}^{{\text{s}}}\) and receiver DCBs from reference station i; \({\text{DCB}}_{{P_{1}  P_{2} ,i}}^{{\text{r}}}\) represents the receiver DCBs at reference station i, and \(n\) indicates the number of reference stations.
In the case of the stochastic parts, the variance of the user’s interpolated ionospheric delays is related to two factors. On the one hand, the noise and multiple paths errors of the reference network may cause the errors to affect the precision of the estimated ionospheric delays. On the other hand, the interpolated error also has an influence on the precision of interpolated ionospheric corrections. Normally, the variance mainly depends on the distance between the reference network and the user station. Thus, the variance \(P_{{\text{u}}}^{{\text{s}}}\) following \(I_{{\text{u}}}^{{\text{s}}}\) can be represented as follows:
where \(P_{{\text{u}}}^{{\text{s}}}\) is the variance of \(I_{{\text{u}}}^{{\text{s}}} ,\) \(\delta_{i}^{{{\text{s}}2}}\) is the precision of the slant ionospheric delay of satellite s visible to reference station i, \({\text{el}}_{i}^{{\text{s}}}\) indicates the elevation angle of satellite s, and \(\mu = 1.04\) mm/km is adopted as the empirical scale factor (Li et al. 2014b; Odijk 2000; Liu and Lachapelle 2002).
Figure 2 shows the geometric relationship between the reference network and the user’s position when using the DIM algorithm to interpolate the slant ionospheric delays. The slant ionospheric correction of a given satellite (s) visible to the user components can be interpolated by utilizing the slant ionospheric delays of the same satellite visible to the reference stations. Moreover, for the user, the processes of generating slant ionospheric correction and variance are carried out epoch by epoch. When the slant ionospheric correction/variance of a given satellite is available for a certain epoch, the user can apply it to improve the convergence performance of PPPRTK.
At the user’s position, the UCPPP model can be enhanced by applying ionospheric correction so that the convergence performance can be improved. The interpolated slant ionospheric corrections derived from the reference network are imported as virtual observations to accelerate the ambiguity resolution of PPP. Specifically, the UCPPP model with additional slant ionospheric constraint information can be expressed as:
where \(\tilde{I}_{{{\text{u}},1,{\text{net}}}}\) and \(\sigma_{{w_{I} }}^{2}\) represent the slant ionospheric correction interpolated from the network component and its corresponding variance, obtained from Eqs. (6) and (7), respectively; \(w_{I}\) denotes the difference between the estimated slant ionospheric delay from the user component and interpolated slant ionospheric correction from the reference network.
Considering the above ionospheric virtual observations, we can extend the UCPPP function model of Eq. (3) to compensate for the variations in the estimated ionospheric delays in the PPPRTK platform of the user components. Similarly, the stochastic model of UCPPP can be extended as well, as presented in Eq. (9):
where \(Q_{{P_{{\text{u}}} P_{{\text{u}}} }}\) and \(Q_{{L_{{\text{u}}} L_{{\text{u}}} }}\) represent the variance–covariance matrix of both the original pseudorange and the carrier phase observations, respectively; \(Q_{{w_{I} w_{I} }}\) represents the variance–covariance matrix of slant ionospheric correction for the user components; and \(E\) is the identity matrix. The notation blkdiag denotes a block diagonal matrix.
PPPRTK platform design
In this study, we used a modified version of the precise point positioning with integer and zerodifference ambiguity resolution demonstrator (PPPWIZARD) software as the PPPRTK platform to carry out the experiments. The PPPWIZARD software was developed by the Centre National d’Etudes Spatiales (CNES) to realize realtime PPP AR (Laurichesse and Privat 2015). The PPPRTK platform was developed in C/C++. This platform mainly contains a network component for slant ionospheric delay estimation and a user component for augmented PPP AR with interpolated slant ionospheric correction. Figure 3 shows the PPPRTK platform’s structure including the network and user component. Because the structure of the network and user components was consistent, except for the estimation strategies of the coordinates and ionosphere parameters, we describe the common functionalities.
First, the configuration file for PPPRTK network data processing needs to be read. Afterwards, the GNSS observations, precise GNSS orbits, clocks, OSB products, the IGS antenna correction file, and the station coordinate file are required as input to the software of the network component. During data processing, epoch by epoch, we fixed the coordinates of the reference stations to improve the accuracy of the slant ionospheric delays and reduce the number of unknown parameters. Second, the measurement cleaning step mainly identifies and removes data errors, including large gross errors and cycle slips. The remaining steps are then carried out. Single point positioning (SPP) is used to compute the initial point coordinates. The propagation step is responsible for resolving the dynamic model (e.g., initial variance, and spectral density) of the state parameters. The observedminuscomputed (OMC) values can be obtained from the measurement model residuals. We applied the residuals of the OMC values to enable the Kalman filter to estimate the floating state vector. Third, UD WL ambiguities are extracted from the floating state parameters, and the SD WL ambiguities are formed by transforming the UD WL ambiguities. When the SD WL ambiguities have been fixed successfully, we can consider the SD WL integer ambiguities to be virtual observations for updating the floating solutions. Similarly, the UD NL ambiguities can be derived from the floating solutions updated with the fixed SD WL ambiguities. When the SD NL ambiguities have been fixed by the LAMBDA algorithm, the state parameters of the floating solutions will be updated with the fixed SD NL ambiguities. Finally, the slant ionospheric delays can be derived from the floating solutions updated with the fixed SD WL and the fixed SD NL ambiguities in succession. At the user end, the station coordinates need to be estimated to investigate the performance of PPPRTK. Slant ionospheric delays interpolated by the DIM method are imported into the PPPRTK user platform epoch by epoch. When the slant ionospheric corrections/variances have been obtained, we can take the slant ionospheric corrections as the virtual observations to enhance the model strength of the floating solutions and improve the convergence performance of PPPRTK.
Results
A mediumscale network
In this part, the data selection and processing strategies for the reference network and the user components are introduced. We then assessed the accuracy of the slant ionospheric corrections by comparing the ionospheric corrections interpolated from the reference network with the user’s results retrieved in the same manner as the network component. Finally, we investigated the convergence performance of PPPRTK in pseudokinematic mode.
Data selection and processing strategies
To validate the convergence performance of PPPRTK, five stations were used for the experiments. These stations belong to the European reference frame (EUREF) Permanent GNSS Network (EPN). Four stations (HETT, SAVU, TORN, and KUU2) were considered to be regional augmentation stations, and the station SOD3 was regarded as a user station. The five stations were equipped with the Javadtype receivers and capable of tracking GNSS satellites. The distribution of the stations is shown in Fig. 4. The average distance between the reference network sites and the user station was about 165 km. This indicates that this network is a mediumscale network.
The geomagnetic Kp index was determined by the GeoForschungsZentrum (GFZ) data services (Matzka et al. 2021a, b). The disturbance storm (Dst) was obtained from the international service of geomagnetic indices (ISGI) (Kauristie et al. 2017). The distribution of the Kp index and Dst from days 082 to 083 is demonstrated in Fig. 5. We can see that the Dst roughly varied from − 30 to 10 nT and the Kp index varied from approximately 0 to 4, which indicates medium ionospheric disturbance during the experimental period (Matzka et al. 2021a).
For PPPRTK data processing for both the network and the user components, the GPS L1/L2 and Galileo E1/E5a observations with a 30s sample interval were used. Furthermore, we applied the final 5 min of the GFZ satellite orbits, 30s satellite clocks, earth rotation parameters (ERPs), and the corresponding OSBs products provided by CNES (Laurichesse and Blot 2016). The absolute antenna phase center was corrected (Schmid et al. 2016). The cutoff elevation angle was set to 10°. An elevationdependent weighting strategy was utilized to reduce the impact of both the atmospheric errors and multipath errors. The standard deviation was 0.3 m and 3 mm for the pseudorange and carrier phase observations in the zenith direction, respectively. The parameter settings of the standard deviation can be considered as an appropriate choice in most cases (Li et al. 2008). An equal weighting strategy was applied to the GPS and Galileo observations. Meanwhile, we corrected the effects of both phase windup and station displacement (Wu et al. 1993; Petit et al. 2010). The dry component of zenith troposphere delays was corrected by applying an a priori Saastamoinen model (Saastamoinen 1972), and the global mapping function (GMF) (Boehm et al. 2006) was employed as a mapping function. Meanwhile, the wet component of the zenith troposphere delays was modeled as a random walk process, in which the spectral density was empirically assumed to be \(5 \times 10^{  5} {\text{m}}/\sqrt {\text{s}}\) (Li et al. 2020).
Figure 6 presents the number of satellites and the position dilution of precision (PDOP) of the user components. The average number of satellites was 10.96 and 19.26 for both the GPSonly and GPS + Galileo observations, respectively. The average values of PDOP were 2.38 and 1.56 for the GPSonly and combined GPS + Galileo observations, respectively. The PDOP values of GPS alone were less than 4 most times, while those of the integrated GPS and Galileo observations were mostly less than 2.
Performance of ionospheric corrections
In this section, the user station SOD3 was regarded as an additional reference station for estimating the UD slant ionospheric delays. The UD slant ionospheric delays of the user station were used for assessing the slant ionospheric corrections. The slant ionospheric corrections were interpolated from the other four reference stations. Unfortunately, UD slant ionospheric delays are usually contaminated by the receiver DCBs. To eliminate the impact of receiver DCBs, it is reasonable to transform the UD slant ionospheric delays into the satellitedifference slant ionospheric delays. This transformation is implemented in two steps for the UD slant ionospheric delays of both the server and the user components simultaneously. Specifically, the first step is to select the reference satellite with the highest elevation angle to find a single difference from other satellites in the same satellite system. The second step is to find the difference between the user’s SD slant ionospheric delays and the networkinterpolated SD slant ionospheric corrections. Both of them are derived from Step 1 and follow the principle of selecting the same satellite pair and the same time. In addition, the accuracy of the slant ionospheric corrections in other satellite systems should be investigated as well.
Based on the above considerations, slant ionospheric corrections derived from the GPS and Galileo constellation can be compared and analyzed. Figure 7 shows the error distribution of the interpolated SD slant ionospheric corrections in detail. For the SD GPS ionospheric residuals, the proportions within 0.15 total electron content units (TECU) and 0.30 TECU were 73.1% and 85.2%, respectively. This means that, converted to L_{1}, 85.2% of the ionospheric residuals were less than 5 cm. The accuracy of the slant ionospheric corrections can significantly accelerate the initialization of the PPP (Geng et al. 2010b). Similarly, proportions of 65.3% and 81.7% for SD Galileo ionospheric residuals were obtained under the conditions of 0.15 and 0.30 TECU, respectively.
Performance of PPPRTK
In this section, the convergence performance of the user components was investigated as follows. To obtain enough samples to assess the convergence performance, the observations were processed every 1 h to assess the convergence performance of PPPRTK. If the SD WL and SD NL ambiguities were fixed successfully, and the positioning errors of both the horizontal and vertical components were less than 4 cm and 10 cm, respectively, the fixed solutions could be achieved successfully (Li et al. 2020). It is worth mentioning that the observations in the first 1 h in all conditions were excluded to ensure that ambiguities at reference sites had been resolved reliably. Specifically, the 50th and 90th percentile curves based on all 46 datasets were used to demonstrate the convergence performance of PPPRTK. The convergence time of PPPRTK is defined as the time to achieve a certain level of positioning accuracy. Specifically, in this work, it means that the horizontal and vertical positioning errors are less than the threshold of 10 cm, respectively. The positioning error is the difference between the estimated positions and true coordinates. What’s more, only when the positioning error of horizontal and vertical components of 20 consecutive epochs after this epoch is less than 10 cm, the PPPRTK can be considered to convergence at this epoch (Li and Zhang 2014).
Figure 8 and Table 2 depict the 50th and 90th percentile convergence performance of the PPPRTK user components. Furthermore, we investigated the convergence performance of both GPS alone and integrated GPS + Galileo. For the 50th percentile situations, the convergence time, in the horizontal and vertical components, respectively, reduced by 1.0 and 1.5 min for the GPSonly observations, and by 0.5 and 1.0 min for the combined GPS + Galileo observations. Compared with GPSonly PPPRTK, PPPRTK based on GPS + Galileo observations reduced the convergence time by an average of 40%. From the results of the 90th percentile, we also found that the convergence time of PPPRTK using GPS observations was 2.5 and 3.0 min in the horizontal and vertical components, respectively. When utilizing GPS + Galileo observations, the PPPRTK convergence times of the horizontal and vertical components improved by 20% and 16.7%, respectively.
The convergence performance of GPSonly PPPRTK was revealed in Psychas and Verhagen (2020). For the 50th percentile positioning errors of the horizontal component, Psychas and Verhagen (2020) took 1.0 and 1.5 min to achieve the 10 cm threshold, in terms of the networks with a spacing of 68 and 115 km. Our results are the same as those of the networks with 68 km and 115km spacing at a 50% confidence level. For the 90th percentile positioning errors, the convergence times of networks with 68 and 115km spacing in the study by Psychas and Verhagen (2020) were approximately 5.0 and 10.0 min, in terms of the horizontal component. By comparing these results, we can see that the 90th percentile horizontal positioning errors of GPSonly PPPRTK can still achieve better than 10cm convergence within 2.5 min when slant ionospheric corrections derived from the network with 165km spacing were utilized. Banville et al. (2014) also investigated fast PPP convergence performance using regional slant ionospheric corrections. Their results demonstrated that when using GPSonly ionospheric corrections derived from the network with 150km spacing, the convergence better than the 10cm threshold could be obtained within 5 min.
It can be seen from the comparison of the results that our results are reliable and valid. However, we also should note that the convergence performance of PPPRTK using regional ionospheric corrections was affected by many factors, such as satellite geometry, the quality of the observations, and ionospheric conditions. As Banville said, the ambiguity resolution of a PPP algorithm should exclude wrongly fixed ambiguities to ensure that ambiguity resolution is accurate, and the precision of ionospheric corrections should actually reflect their deficiencies in UCPPP model to enhance the UCPPP model strength to accelerate the ambiguity fixing.
A smallscale network
In this section, first, we processed a National Oceanic and Atmospheric Administration (NOAA) Continuously Operating Reference Stations (CORS) Network (NCN), whose processing strategies are the same as those of the network with 165km spacing. We then evaluated the accuracy of the slant ionospheric corrections interpolated from the reference network. Finally, the convergence performance of PPPRTK was implemented for validation in pseudokinematic mode.
Data selection and processing strategies
To investigate the convergence performance of PPPRTK, five stations were utilized to process the GNSS data. Four reference stations (MNGR, MNSB, MNMR, and MNCL) were considered as reference stations for generating slant ionospheric corrections, and the MNAN station was regarded as the user station. The five stations were equipped with Trimbletype receivers and capable of tracking GNSS satellites. The distribution of the GNSS network is shown in Fig. 9. We applied 2 days (days 082 and 083 of 2021) of GPS L1/L2 and Galileo E1/E5a observations with a 30s sample to carry out PPPRTK in pseudokinematic mode. The average distance between the reference network sites and the user station was about 50 km. The network of this scale indicates a smallscale network.
Performance of ionospheric corrections
In this section, the user station MNAN was considered as an additional reference station for obtaining the UD slant ionospheric delays. The slant ionospheric delays of the user station were used to evaluate the UD slant ionospheric corrections. The slant ionospheric corrections were interpolated from the reference network. Due to the receiver DCBs remaining in the ionospheric delays, we used the SD operators on the ionospheric delays to remove the impacts of the receiver DCBs. The specific assessment method is described in the previous section.
The error distribution of the interpolated SD ionospheric corrections is depicted in Fig. 10. In terms of the SD slant ionospheric residuals of the GPS constellation, the proportion within 0.15 TECU is 92.2%, while that within 0.30 TECU is 95.9%. In the case of the Galileo scenario, proportions of 75.4% and 82.8% were obtained under the conditions of 0.15 and 0.30 TECU, respectively. Comparing Figs. 7 and 10, we can see that the proportions of SD ionospheric residuals in smallscale networks are higher than those of mediumscale networks under the conditions of 0.15 and 0.30 TECU, whether the GPS and Galileo constellation is used. This may be because the accuracy of the ionospheric delays has a strong correlation with the distance between stations (Liu and Lachapelle 2002). The longer distance between stations, the weaker the correlation of the ionospheric delays (Gao et al. 2021). Larger modeling errors of the ionospheric delays may be generated in a largerscale network. This may be the reason why the proportions of SD ionospheric residuals generated from the mediumscale network were lower than those from the smallscale network. Of course, networks with different scales may require similar ionospheric conditions.
From Fig. 10, we can also find another situation, which the proportion of GPS SD slant ionospheric residuals in a certain range is higher than that of Galileo. A similar situation exists in Fig. 7, but their difference in Fig. 7 is slightly smaller than that in Fig. 10. To further study the reasons behind this phenomenon, we analyze the number of both ionospheric delays and fixed SD NL ambiguities, whether for reference network and user components. Due to the limited length of the article, we only present and analyze the limited results of both reference network and user components. Other situations are generally the same as those shown in this paper.
From Figs. 11 and 12, we can find that the number of Galileo ionosphere is less than that of GPS, whether for reference network station MNMR or user station MNAN. Furthermore, the number of Galileo NL resolved ambiguities is also less than that of the ionosphere. As we know, the more the number of resolved ambiguities and the better spatial geometry, the more significant the effect of improving the accuracy of positioning and other parameters to be estimated in the UCPPP model. On the contrary, if the number of resolved ambiguities is small, the accuracy of estimated parameters in the fixed solutions may not be well guaranteed. Hence, comparing Figs. 10, 11, and 12, it is suggested that the main reason for the large ionospheric residuals of Galileo is mainly due to the insufficient resolved number of NL ambiguities resulting in low ionospheric accuracy. Of course, many other potential factors that affect ambiguity fixing, e.g., data quality of Galileo, the accuracy of Galileo orbit/clock products, the corrections of receiver’s PCOs and PCVs, and the defined weight strategies between GPS observations and Galileo observations. Finally, we believe that these are temporary problems. With the completion of Galileo’s global network deployment and the further improvement of corresponding models and algorithms, the performance of Galileo’s ionospheric residuals will be close to GPS.
Performance of PPPRTK
We took the 50th and 90th percentile positioning errors of both the horizontal and vertical components as indicators to investigate the convergence performance of PPPRTK for GPS alone and integrated GPS + Galileo observations. Figure 13 and Table 3 show the convergence performance of PPPRTK for the 50th and 90th percentiles of the horizontal and vertical positioning errors in detail. For the 50th percentile scenario, the integrated GPS + Galileo observations had no obvious advantage over the GPSonly observations in terms of the convergence performance of the horizontal and vertical components. This indicates that the constraints of ionospheric corrections can significantly reduce the correlation between the positioning parameters and other estimated parameters in GPSonly PPPRTK of the user components. Hence, the Galileo observations did not reduce the convergence time at the 50% confidence level. On the contrary, the horizontal and vertical convergence time reduced from 2.0 min for GPSonly PPPRTK to 1.5 min for integrated GPS + Galileo PPPRTK at the 90% confidence level. The convergence time could be shortened by 25% by using GPS and Galileo observations.
To investigate the convergence performance of PPPRTK in networks with different scales, we compared the PPPRTK convergence time between the mediumscale network and the smallscale network. As far as the 90% confidence level was concerned, the average convergence time of the smallscale network was less than that of the mediumscale network. Therefore, it can be suggested that the convergence time of PPPRTK is related to the scale of the reference network. The larger scale of the reference network, the longer the convergence time of the user components (Psychas and Verhagen 2020). The relationship between the convergence time of the user and the scale of the network has also been verified in analyses of the accuracy of the ionospheric corrections derived from networks with different scales (Gao et al. 2021). In terms of the largerscale network, the convergence time was affected by the accuracy of the interpolated slant ionospheric corrections. Overall, although the scale of the reference network affected the convergence performance of PPPRTK, our results suggest that the GPSonly PPPRTK could achieve convergence in the horizontal direction within 2.0 and 2.5 min and the integrated GPS + Galileo PPPRTK could achieve convergence in the horizontal direction within 1.5 and 2.0 min for the smallscale network and the mediumscale network, respectively.
Discussion
In this study, we investigated the convergence performance of GPS + Galileo PPPRTK using two networks with different scales. As far as the accuracy assessment of the interpolated ionospheric corrections is concerned, for the network with 165km spacing, the proportion of the GPS SD ionospheric residuals within 0.30 TECU was 85.2%, while that of the Galileo SD ionospheric residuals was 81.7%. For the network with 50km spacing, the proportion of GPS SD ionospheric residuals within 0.30 TECU was 95.9%, while that of the Galileo SD ionospheric residuals was 82.8%. The difference in the proportions of SD ionospheric residuals between the 165km network and the 50km network was associated with the ionospheric modeling errors. The errors mainly depend on the distance between stations (Xiang et al. 2020). Meanwhile, it is also noted that the ionospheric parameters not only have uncertain random variations but also contain the receiver’s DCBs. When different receiver types are used for the stations in the reference network, the interpolated slant ionospheric delays derived from can be affected due to the large differences of receiver’s DCBs. Therefore, these ionospheric delays containing the receiver’s DCBs may not be suitable for direct interpolation of ionospheric delays, because the relationship between the spatiotemporal variation characteristics of DCBs and the ionospheric delays needs further research. From the perspective of ionospheric modeling, the impact of the receiver’s DCBs can be eliminated by using the SD ionospheric delays between satellites. However, as we know, the reference satellite can only be viewed by the reference network and user station within a certain range. When it exceeds a certain range, this method may be invalid for the ionospheric modeling of widearea PPPRTK. Hence, to maintain a high degree of selfconsistency between the reference network and user component of PPPRTK, the best strategy to resolve the receiver’s DCBs is to apply the global ionospheric maps (GIMs), which are considered initial values to constrain the ionospheric parameters in UCPPP model. Therefore, the receiver’s DCBs can be effectively separated from the slant ionospheric delays. Correspondingly, when the user utilizes the interpolated slant ionospheric delays, the receiver’s DCBs can also be estimated in the UCPPP model, which does not affect the model strength of PPPRTK. In addition to the effect of the receiver’s DCBs, the condition of the observation, reference network scales may affect the degree of agreement between interpolated slant ionospheric delays derived from the reference network and selfestimated slant ionospheric delays estimated from user components. On the other hand, in this study, the DIM uses the empirical scale factor to compensate for the effect of interstation distance on the accuracy of the interpolated ionospheric delays. Li et al. (2014b) gave a variable range of empirical scale factors from 0.3 to 3 mm/km. Odijk (2000) took 0.57 mm/km as the scale factor to research the Californian network. However, the empirical accuracy of interpolated ionospheric corrections may not effectively mitigate the impact of ionospheric delays in the UCPPP model. Hence, it is necessary to propose an ionospheric modeling method that is suitable for various networks of different scales and eliminates the impact of the receiver’s DCBs. More importantly, this model should adequately reflect the random variation characteristics of the ionospheric delays.
In terms of the convergence performance of PPPRTK, for the 165km network, it took 2.5 and 2.0 min for the GPSonly and integrated GPS + Galileo observations to achieve the 10cm threshold for the 90th percentile horizontal positioning errors. Using the slant ionospheric corrections derived from the network with 50km spacing, the GPSonly, and integrated GPS + Galileo PPPRTK achieved convergence in the horizontal direction within 2.0 and 1.5 min at the 90% confidence level. The PPPRTK convergence time was further reduced by utilizing the GPS and Galileo observations together. Meanwhile, it has been noted that when the scale of the network becomes larger, the convergence time of PPPRTK will become longer to some extent. This has already been verified in Psychas and Verhagen (2020). The GPSonly PPPRTK using regional ionospheric corrections derived from the network with 165km spacing achieved convergence in the horizontal direction within 2.5 min at the 90% confidence level. Similar results have also been found in Banville et al. (2014), which indicates our results are reliable. This suggests that our results may provide a reference for studying the convergence performance of multiGNSS PPPRTK based on networks with different scales.
Even though the expected results could be found, our study only concentrated on validation of the results by utilizing limited GPS/Galileo observations from two networks with different scales under medium ionospheric disturbance. Ionospheric delays have many complicated characteristics in time and space, which are not still fully known at present. Hence, new ideas require to be proposed for ionospheric modeling, especially for the widearea slant total electron content (STEC) modeling algorithm. Furthermore, it is expected that the convergence performance of PPPRTK can be further improved by using multiGNSS and multifrequency observations. Considering the above analysis, the modeling algorithm of STEC and the potential of multiGNSS and multifrequency for PPPRTK should be comprehensively investigated in the future.
Conclusions
This contribution mainly investigates the convergence performance of PPPRTK by using GPS and Galileo observations. To this end, the convergence performance of PPPRTK was assessed by utilizing the GPS/Galileo observations from two networks with a large difference in their scale.
For the network with an average distance of about 165 km, 85.2% of the SD GPS ionospheric residuals were within 0.30 TECU, while 81.7% of the SD Galileo ionospheric residuals were within 0.30 TECU. In terms of the 50th percentile, the PPPRTK convergence times in the horizontal and vertical directions were reduced from 1.0 and 1.5 min for the GPS alone observations to 0.5 and 1.0 min for the integrated GPS + Galileo observations. An average improvement of 40% could be obtained. Similarly, for the 90th percentile positioning errors of the horizontal and vertical components, the convergence times to be reduced from 2.5 and 3.0 min for the GPSonly observations to 2.0 and 2.5 min for the integrated GPS + Galileo observations, with an average improvement of 18.1%.
For the network with an average distance of about 50 km, 95.9% of the SD GPS ionospheric residuals were within 0.30 TECU, while 82.8% of the SD Galileo ionospheric residuals were within 0.30 TECU, respectively. The 90th percentile positioning errors of the horizontal and vertical components reduced the convergence times from 2.0 and 2.0 min for the GPSonly observations to 1.5 and 1.5 min for the integrated GPS + Galileo observations. An average improvement of 25% could be achieved.
Whether it is the accuracy of slant ionospheric delays or the convergence performance of PPPRTK, the 50km network showed obvious advantages. This is mainly because of the strong correlation between the ionosphere and the scale of the reference network. Meanwhile, it is noted that the integrated GPS and Galileo observations could further reduce the convergence time of PPPRTK for the networks with 50 and 165km spacing.
Availability of data and materials
The precise orbit and clock products from GFZ and CNES are obtained at ftp://ftp.gfzpotsdam.de/pub/GNSS/products/mgex/ and https://www.pppwizard.net/products/POST_PROCESSED/; multiGNSS observations are available through EUREF and NCN data centers (ftp://ftp.epncb.oma.be/pub/obs/; https://geodesy.noaa.gov/corsdata/rinex/).
Abbreviations
 PPP:

Precise point positioning
 AR:

Ambiguity resolution
 PPPRTK:

PPP realtime kinematic
 GPS:

Global Positioning System
 GNSS:

Global Navigation Satellite Systems
 BDS:

BeiDou Navigation Satellite System
 RMS:

Rootmeansquare
 Galileo:

Galileo Satellite Navigation System
 PCOs:

Phase center offsets
 PCVs:

Phase center variations
 IF:

Ionospheric free
 DCBs:

Differential code biases
 NL:

Narrowlane
 WL:

Widelane
 OSBs:

Observables specific signal biases
 UPDs:

Uncalibrated phase delays
 SD:

Singledifference
 LAMBDA:

Leastsquare ambiguity decorrection adjustent
 ILS:

Integer leastsquare
 UD:

Undifference
 DIM:

Distancebased linear interpolation method
 PPPWIZARD:

Precise point positioning with integer and zerodifference ambiguity resolution demonstrater
 CNES:

Centre National d’Etudes Spatiales
 OMC:

Observedminuscomputed
 EUREF:

European reference frame
 EPN:

European reference frame Permanent GNSS Network
 GFZ:

GeoForschungsZentrum
 Dst:

Disturbance storm
 ISGI:

International service of geomanetic indices
 ERPs:

Earth rotation parameters
 GMF:

Global mapping function
 PDOP:

Position dilution of precision
 TECU:

Total electron content units
 NOAA:

National Oceanic and Atmospheric Administration
 CORS:

Continuously Operating Reference Stations
 NCN:

National Oceanic and Atmospheric Administration Continuously Operating Reference Stations Network
 STEC:

Slant total electron content
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Acknowledgements
The authors are very grateful to thank three anonymous reviewers of this paper for their meaningful suggestions and comments. The GFZ, CNES Analysis Center, EUREF Permanent GNSS Network, and NCN are also appreciated for providing access to multiGNSS products and multiGNSS observations.
Funding
This research was funded by the National Science Fund for Distinguished Yong Scholars (No. 41825009), the Changjiang Scholars Program.
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YZ performed the data processing and drafted the manuscript. ZX discussed and analyzed the data, critically revised the manuscript, and proofread the submission. Both authors read and approved the final manuscript.
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YZ is a Ph.D. candidate of Wuhan University. His current research is MultiGNSS and Multifrequency PPPRTK and regional ionosphere modeling. ZX is a professor of Wuhan University. His current research involves GNSS precise point positioning and GNSS/INS.
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Yan, Z., Zhang, X. Assessment of the performance of GPS/Galileo PPPRTK convergence using ionospheric corrections from networks with different scales. Earth Planets Space 74, 47 (2022). https://doi.org/10.1186/s40623022016029
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DOI: https://doi.org/10.1186/s40623022016029
Keywords
 PPPRTK
 GNSS
 Slant ionospheric corrections
 Total electron content unit